The Cosmic Neutrino Background Anisotropy - Linear Theory

Details The Cosmic Neutrino Background Anisotropy - Linear Theory The Cosmic Neutrino Background Anisotropy - Linear Theory

2009-10-26

arxiv.org/abs/0910.4578v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

16 pages, 8 figures, JCAP format

Scientific paper

The cosmic neutrino background anisotropy is calculated for massive neutrino
states by solving the full Boltzmann equation. The effect of weak gravitational
lensing, including the Limber approximation, is also derived for massive
particles, and subsequently applied to the case of massive neutrinos.

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